In general relativity (GR), energy conservation is defined locally rather than globally, leading to the conclusion that energy can appear to increase with the universe's expansion and the constant density of dark energy. The discussion highlights that while energy is conserved in closed systems, GR lacks a global conservation law due to the failure of Gauss's law in four-dimensional space. This means that the universe can theoretically create or annihilate energy, complicating traditional energy calculations. Additionally, the energy density associated with the cosmological constant remains constant, while the volume of space expands, resulting in an overall increase in total energy. Ultimately, GR does not provide a framework for global energy conservation, particularly in dynamic cosmological contexts.